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[ci skip] add documentation, changelog, and a warning
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docs/source/changelog.rst

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@@ -90,6 +90,10 @@ starting models has been recalculated with a more stringent stopping condition,
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and now all pre-computed ZAMS models have a central hydrogen mass fraction very
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near 0.697.
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The ``fixed_Teff``, ``fixed_Tsurf``, ``fixed_Psurf``, and ``fixed_Psurf_and_Tsurf``
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atmosphere options have been reimplemented, although we caution users that their
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implementation might conflict with mlt_option = ``TDC``.
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Changes in r23.05.1
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===================
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star/defaults/controls.defaults

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! ~~~~~~~~~~
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! Controls how the surface temperature Tsurf and pressure Psurf are evaluated when
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! setting up outer boundary conditions
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! setting up outer boundary conditions. We caution that the use of ``'fixed_'`` atmosphere
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! options might conflict with mlt_option = ``TDC``.
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! + ``'T_tau'``:
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! set Tsurf and Psurf by solving for the atmosphere structure given a T(tau) relation.
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! + ``'fixed_Psurf_and_Tsurf'`` :
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! get value of Psurf from control parameter ``atm_fixed_Psurf``.
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! get value of Tsurf from control parameter ``atm_fixed_Tsurf``.
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! see the ``conductive_flame`` test_suite for an example of
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! this boundary condition implemented via the ``other_surface_PT`` hook.
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! ::
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star/test_suite/conductive_flame/README.rst

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The inner boundary is at r = 0. The outer boundary has a fixed
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temperature and a fixed pressure equal to the initial pressure of the
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material. This is achieved via the ``use_other_surface_PT`` hook.
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material. This is achieved via the ``use_other_surface_PT`` hook, but
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can also be done using the ``fixed_Psurf_and_Tsurf`` atmosphere option.
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After an initial transient, the entire flame structure, approximately
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isobaric, propagates into the upstream fuel with a unique speed and
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.. |Schwab2020| replace:: `Schwab et al. (2020) <https://ui.adsabs.harvard.edu/abs/2020ApJ...891....5S/abstract>`__
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Last-Updated: 2021-06-21 (mesa b2364463) by Josiah Schwab
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Last-Updated: 2021-06-21 (mesa b2364463) by Josiah Schwab, + documentation 2024-01-22 EbF
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